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<ri:Resource created="2021-01-27T08:06:33Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Properties of LMC star clusters</title><shortName>J/MNRAS/499/4114</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/499/4114</identifier><altIdentifier>doi:10.26093/cds/vizier.74994114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gatto M.</name></creator><creator><name>Ripepi V.</name></creator><creator><name>Bellazzini M.</name></creator><creator><name>Cignoni M.</name></creator><creator><name>Cioni M.-R.L.</name></creator><creator><name>Dall'Ora M.,Longo G.</name></creator><creator><name>Marconi M.</name></creator><creator><name>Schipani P.</name></creator><creator><name>Tosi M.</name></creator><date role="Updated">2024-08-21T20:16:26Z</date><date role="Created">2021-01-27T08:06:33Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>magellanic-clouds</subject><subject>open-star-clusters</subject><description>The YMCA (Yes, Magellanic Clouds Again) and STEP (The SMC in Time: Evolution of a Prototype interacting late-type dwarf galaxy) projects are deep g, i photometric surveys carried out with the VLT Survey Telescope (VST) and devoted to study the outskirts of the Magellanic System. A main goal of YMCA and STEP is to identify candidate stellar clusters and complete their census out to the outermost regions of the Magellanic Clouds. We adopted a specific overdensity search technique coupled with a visual inspection of the colour-magnitude diagrams to select the best candidates and estimate their ages. To date, we analysed a region of 23 square degrees in the outskirts of the Large Magellanic Cloud, detecting 85 candidate cluster candidates, 16 of which have estimated ages falling in the so-called age gap. 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